Tag: mars science lab

News from Mars: Curiosity Arrives at Mount Sharp

curiosity-mars-self-portrait-crop-640x353After two years exploring the Martian surface, the Curiosity Rover has finally reached its primary science destination – the foot of Mount Sharp, officially known as Aeolis Mons. Now that it’s there, it will begin its ascent of the rock formation, drill into rocks and analyze the different strata in the hopes of learning more about the history of the Red Planet. This is an event a long time in the making, and may prove to yield some of the greatest scientific discoveries ever made.

Located in the heart of the Gale Crater, Mount Sharp is like a layer cake, holding a chronology of past events reaching back billions of years. Because of this, it is an ideal place to find evidence that the Martian surface and atmosphere were once capable of supporting life. It took two years and one month for Curiosity reach the foot of this mountain, which lies some 5500 meters (18,000 feet) above the floor of Gale Crater.

MarsCuriosityTrek_20140911_AThe mountain is the central peak in a crater that measures 154 km/96 miles in diameter and which was formed when a meteor impacted the surface between 3.5 and 3.8 billion years ago. Beyond a certain size, and depending on the gravity of the planet, craters like this all have a central peak. But Mount Sharp represents something much more, otherwise NASA and the Jet Propulsion Laboratory wouldn’t be bothering with it.

Basically, Mars scientists believe that after its creation, the Gale crater was completely filled with sedimentary material from a series of huge floods, or by dust and ice deposits like those that happened at the Martian polar caps. The deposition over 2 billion years left a series sedimentary layers that filled the crater. Following the deposition of the layers, there was a long period of erosion which has finally led to the condition of the crater today.

mountsharp_galecraterThe erosion by some combination of aeolean (wind) forces and water (additional flooding), scooped out the huge crater, re-exposing most of the original depth. However, covering the original central peak are many sedimentary layers of debris. Gale crater’s original central peak actually remains completely hidden and covered by sedimentation. And it is this that attracted scientists with the Curiosity rover to the base of Mount Sharp.

Within the sedimentary layers is a sequential record of the environmental conditions on Mars going back over 2 billion years. While at the base, Curiosity will be able to examine the oldest sedimentary layers; but as it climbs the flanks of the mountain, it will be able to step forward in time. Each layer and its age will reveal information such as how much water was present, whether the water was alkaline or acidic, if there is any organic compounds.

john_klein_curiosity-2The discovery of organic compounds on Mount Sharp could be “Earth shaking”, since the discovery of organics is of very high importance to this mission. Already, over the two year trek, Curiosity has seen numerous signs of the flow of water and sedimentation. Interestingly enough, evidence began to turn up way back in Yellowknife Bay — one of its first destinations, which it visited almost two years ago. But as of yet, signs of organic compounds have remained illusive.

What’s more, Curiosity sadly lacks the necessary equipment to look for evidence of microbial fossils or other signatures of life. Fortunately, the next rover – the Mars 2020 rover – will be equipped with the necessary tools to work out whether Mars ever harbored life. In any case, because of the lack of organic compounds in Yellowknife, NASA decided to continue to Mount Sharp, which is currently the best place to dig up scientific data about Mars’ past.

MSL_TraverseMap_Sol0743-2048Curiosity is currently at the base of Mount Sharp, in a region called the Pahrump Hills, where it will continue on to the Murray Formation. Once there, it will take a drill sample of some rock and then continue up Mount Sharp towards the Hematite Ridge where two drill sites await. This farthest site is about 8 km (5 mi) away from its present position, and Curiosity has driven only 9 km since it landed in 2012. So there’s plenty of trekking and work ahead!

One of the greatest challenges is finding a path that will reduce the stress on Curiosity’s wheels, which have been put through some serious wear and tear in the past two years. Because of this, the rover is being driven in reverse for the time being, and the team is looking the path with the least amount of sharp rocks. However, the Mars Curiosity remains confident that the mobility system will be capable of surviving the ten year life span of the rover’s power supply.

And be sure to check out this “Curiosity Rover Report” that talks about this historic accomplishment, courtesy of NASA’s Jet Propulsion Laboratory:

Sources: universetoday.com, extremetech.com, jpl.nasa.gov, space.com

News from Mars: Martian Water and Earth Organisms

curiosity_peakThis August, the Curiosity Rover will be celebrating its second anniversary of roving around the Red Planet. And ever since it made landfall, Curiosity and the Mars Science Laboratory has repeatedly uncovered signs that Mars was once very like Earth. Basically, it has become undeniable that water once flowed freely over the surface of this barren and uninhabitable world. And this finding, much to the delight of futurists and sci-fi enthusiasts everywhere, is likely to pave the way for human settlement.

Liquid water disappeared from Mars’ surface millions of years ago, leaving behind tantalizing clues about the planet’s ancient past—clues that the MSL has been deciphering for the past 22 months. This began last year when Curiosity found rounded pebbles in the Glenelg region, an indication that a stream once flowed at the site. This was followed by the discovery of rocky outcroppings where the remains of an ancient stream bed consisting of water-worn gravel that was washed down from the rim of Gale Crater.

mountsharp_galecraterThe rover has since moved to a location about 6.5 kilometers (4 miles) away from the Gale Crater landing site, where scientists expect to make even more discoveries. The new location is named Kimberly, after a region of northwestern Australia. As Dawn Sumner, a UC Davis geology professor and co-investigator for NASA’s Mars Science Laboratory team, explained:

Our findings are showing that Mars is a planet that was once a whole lot like Earth. All the rocks we’ve seen on this mission are sediments that have been deposited by water. We’ve found almost no sandstone deposited by wind.

Sumner is working from Curiosity mission control at NASA’s Jet Propulsion Laboratory in Pasadena while on sabbatical from UC Davis, exploring whether the planet ever had an environment capable of supporting microbial life. She is also one of several UC scientists and engineers who have been vital to the success of the Curiosity mission, which is part of NASA’s long-term plan to pave the way for sending astronauts to Mars.

Living-Mars.2In that vein, research continues here on Earth to see exactly what kind of life can survive in the harsh Martian environment. And now,  research suggests that methanogens – among the simplest and oldest organisms on Earth – could survive on Mars. These microorganisms are typically found in swamps and marshes, where they use hydrogen as their energy source and carbon dioxide as their carbon source to produce methane (aka. natural gas).

As an anaerobic bacteria, methanogens don’t require require oxygen or organic nutrients to live, and are non-photosynthetic. Hence, they would be able to exist in sub-surface environments and would therefore be ideal candidates for life on Mars. Rebecca Mickol, a doctoral student in space and planetary sciences at the University of Arkansas, subjected two species of methanogens to Martian conditions to see how they would fair on the Red Planet.

methanogens485These strains included Methanothermobacter wolfeii and Methanobacterium formicicum, both of which survived the Martian freeze-thaw cycles that Mickol replicated in her experiments. This consisted of testing the species for their ability to withstand Martian freeze-thaw cycles that are below the organisms’ ideal growth temperatures. As she explained it:

The surface temperature on Mars varies widely, often ranging between minus 90 degrees Celsius and 27 degrees Celsius over one Martian day. If any life were to exist on Mars right now, it would at least have to survive that temperature range. The survival of these two methanogen species exposed to long-term freeze/thaw cycles suggests methanogens could potentially inhabit the subsurface of Mars.

Mickol conducted the study with Timothy Kral, professor of biological sciences in the Arkansas Center for Space and Planetary Sciences and lead scientist on the project. She presented her work at the 2014 General Meeting of the American Society for Microbiology, which was held from May 17th to 20th in Boston.

maven_atmosphereThe two species were selected because one is a hyperthermophile, meaning it thrives under extremely hot temperatures, and the other is a thermophile, which thrives under warm temperatures. Since the 1990s, Kral has been studying methanogens and examining their ability to survive on Mars. In 2004, scientists discovered methane in the Martian atmosphere, and immediately the question of the source became an important one. According to Kral:

When they made that discovery, we were really excited because you ask the question ‘What’s the source of that methane?. One possibility would be methanogens.

Understanding the makeup of Mars atmosphere and ecology is another major step towards ensuring that life can exist there again someday. From Red Planet, to Blue Planet, to Green Planet… it all begins with a fundamental understanding of what is currently able to withstand the Martian environment. And once this foundation is secured, our ecologists and environmental engineers can begin contemplating what it will take to create a viable atmosphere and sustainable sources of water there someday.

terraformingSources: phys.org, (2)

Mission to Europa: NASA now Taking Suggestions

europa_moon_IoJupiter’s moon of Europa has been the subject of much speculation and intrigue ever since it was first discovered by Galileo in 1610. In addition to having visible sources of (frozen) surface water and a tenuous oxygen atmosphere, it is also believed to boast interior oceans that could very well support life. As evidence for this mounts, plans to explore Europa using robot landers, miners, submersibles, or even manned missions have been floated by various sources.

However, it was this past December when astronomers announced that water plumes erupting 161 kilometers (100 miles) high from the moon’s icy south pole that things really took a turn. It was the best evidence to date that Europa, heated internally by the powerful tidal forces generated by Jupiter’s gravity, has a deep subsurface ocean. In part because of this, NASA recently issued a Request for Information (RFI) to science and engineering communities for ideas for a mission to the enigmatic moon. Any ideas need to address fundamental questions about the subsurface ocean and the search for life beyond Earth.

europa-lander-2This is not the first time that NASA has toyed with the idea of investigating the Jovian moon for signs of life. Last summer, an article by NASA scientists was published in the peer-reviewed journal Astrobiology, which was entitled “Science Potential from a Europa Lander“. This article set out their research goals in more detail, and speculated how they might be practically achieved. At the time, the article indicated NASA’s ongoing interest, but this latest call for public participation shows that the idea is being taken more seriously.

This is positive news considering that NASA’s planned JIMO mission – Jupiter Icy Moon Orbiter, which was cancelled in 2005 – would be taking place by this time next year. Originally slated for launch between May and January of 2015/16, the mission involved sending a probe to Jupiter by 2021, which would then deploy landers to Callisto, Ganymede, Io and Europa for a series of 30 day studies. At the end of the mission in 2025, the vehicle would be parked in a stable orbit around Europa.

JIMO_Europa_Lander_MissionJohn Grunsfeld, associate administrator for the NASA Science Mission Directorate, had the following to say in a recent press release:

This is an opportunity to hear from those creative teams that have ideas on how we can achieve the most science at minimum cost… Europa is one of the most interesting sites in our solar system in the search for life beyond Earth. The drive to explore Europa has stimulated not only scientific interest but also the ingenuity of engineers and scientists with innovative concepts.

By opening the mission up to public input, it also appears that NASA is acknowledging the nature of space travel in the modern age. As has demonstrated with Chris Hadfield’s mission aboard the ISS, the Curiosity rover, as well as private ventures such as Mars One, Inspiration Mars, and Objective Europa  – the future of space exploration and scientific study will involve a degree of social media and public participation never before seen.

europa_reportThe RFI’s focus is for concepts for a mission that costs less than $1 billion, but will cover five key scientific objectives that are necessary to improve our understanding of this potentially habitable moon. Primarily, the mission will need to:

  1. Characterize the extent of the ocean and its relation to the deeper interior
  2. Characterize the ice shell and any subsurface water, including their heterogeneity, and the nature of surface-ice-ocean exchange
  3. Determine global surface, compositions and chemistry, especially as related to habitability
  4. Understand the formation of surface features, including sites of recent or current activity, identify and characterize candidate sites for future detailed exploration
  5. Understand Europa’s space environment and interaction with the magnetosphere.

Although Europa has been visited by spacecraft and imaged distantly by Hubble, more detailed research is necessary to understand the complexities of this moon and its potential for life. NASA’s Galileo spacecraft, launched in 1989 was the only mission to visit Europa, passing close by the moon fewer than a dozen times. Ergo, if we’re ever to determine conclusively whether or not life exists there, we’re going to have to put boots (robotic or human) onto the surface and start digging!

To read the full Decadal Survey report on NASA’s website, click here.

Sources: universetoday.com, IO9.com, science.nasa.gov

News From Mars!

An interesting slew of news has been coming from NASA recently, courtesy of the Curiosity Rover and its mission to Mars. First, there was the announcement by John Grotzinger on NPR radio that Curiosity’s science team had discovered something potentially “earth-shattering” on the Red Planet, which came just two days ago. Since then, researchers over at NASA have been keeping a tight lip on what that might be, though it seems to be taking an extraodinary effort to do so. One can only imagine what they’re dying to tell us…

But it seems more stories are coming in the wake of this. First, there was the revelation by the Curiosity Rover that Mars radiation levels, once thought to be problematic for life, are actually safe for humans. According to Don Hassler, the principal investigator on Curiosity’s Radiation Assessment Detector instrument (RAD), Curiosity determined that “the Mars atmosphere is acting as a shield for the radiation on the surface and as the atmosphere gets thicker, that provides more of a shield and therefore we see a dip in our radiation dose.”

Apparently, the levels are equal to what astronauts deal with on the International Space Station, which means people in suits will be able to walk on the Red Planet safely once a manned mission is mounted. Knowing that they can conduct surveys on the surface without additional radiation shields should prove to be a boon for colonization as well. More settlers will certainly be drawn to Mars now that they know they can settle in without having to worry about little things like radiation sickness or mutations!

Third, there was the news that in the wake of making its “one for the history books” discovery, that Curiosity has finished collecting and analyzing soil samples and is preparing to move on. The final checks and preps were made amidst ethereal whirlwinds and twisters, which are characteristic of the region known as the “Gale Crater”, where it has been conducting its research for the past month. The rover is now being prepared to move on in search of suitable targets for a compact rock drill, the final major sample acquisition system to be tested.

Ashwin Vasavada, the deputy project scientist for the Mars Science Laboratory rover at the Jet Propulsion Laboratory in Pasadena, Calif, had this to say on the next phase of the mission: “We still would like to get a little further into this Glenelg region where we see this diversity of rocks and layered rocks and other really interesting terrain. And then we still have a goal in the next month or two of doing the big U-turn and heading up to Mount Sharp.”

Mount Sharp is a 3-mile-high mound of layered terrain that sits in the center of the Gale Crater, where Curiosity is expected to spend the bulk of its planned two-year mission. In the meantime, the research team needs to go over all the information Curiosity has sent back, including an ongoing analysis of the martian weather.

On top of all that, there’s still the matter of that “earth shaking news”. How about it NASA? You too, Grotzinger? We’re ready and waiting… how much more time do your researchers need before they’re sure and are free to break the news they are so clearly dying to share? I still say its organic molecules, but what do I know?

Source: news.cnet.com

More News From Curiosity!

Last weekend, Curiosity began conducting the “scooping” portion of its mission; in essence, taking samples of Martian soil from the area known as the Rocknest, and examining them using it’s array of sensors. In the course of doing so, it came across another interesting find – a series of shiny objects, not unlike the small shard of plastic it had discovered ten days earlier.

However, NASA indicated after a preliminary examination that unlike that shard of plastic, these objects did not come from Curiosity itself. According to John Grotzinger, a project scientist with the Mars Science Laboratory, “As the science team thought about it more and more, the bright object is about the same size as the granules that it’s in and it is not uniformly bright. We went back and forth, and the majority of the science team thinks this is indigenous to Mars.”

One hypothesis is that the specks are natural geologic material that might have a broken-off from larger crystalline formations, known as a cleavage, and became dispersed through the soil. These crystalline minerals are more adept at reflecting sunlight than the soil that contains them, hence why they appeared after Curiosity’s scooping exposed them to Martian daylight.

According to Grotzinger, the next step is to examine them using the ChemCam, “a remote sensing tool that has spectacular spatial resolution, and aim it right on that fleck. Then we’ll aim it on another darker grain and try to decide if it is a different class of mineral.” And that’s just one of the fancy tools it will be employing. Another is the Chemistry and Mineralogy (CheMin) instrument, which analyzes samples of dirt to determine what minerals the sample contains. The team announced at a press conference the rover successfully placed a small sample of soil inside this sensor, and expects results in short order.

Stay tuned for more new from Mars!

Source: Universe Today